BD+25_1981
/A.M.Boesgaard(2007)/ /T.Gehren et al.(2006)/
Beryllium in Ultra-Lithium-Deficient Halo Stars:The Blue Straggler Connection
Teff : 6811+-40 | log g : 4.00+-0.40 | vturb : 1.5 |
Original Data | Converted Data Asplund et al. (2009) | |||||||
---|---|---|---|---|---|---|---|---|
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li | N/A | ... | ... | <1.75 | <-1.51 | <-0.25 | <1.75 | Li |
Be | N/A | ... | ... | -0.90 | -2.28 | -1.02 | -0.90 | Be |
Fe | N/A | -1.26+-0.10 | ... | ... | -1.26+-0.10 | ... | 6.24+-0.10 | Fe |
Right Ascension : 08 44 24.69 | Declination : +24 47 47.7 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2004-11-07 | N/A | KECKHIRES | 46000 | 170 | 30 | N/A |
2005-01-31 | N/A | KECKHIRES | 46000 | 160 | 30 | N/A |
Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
Teff : 6820 | log g : 4.11+-0.23 | vturb : 2.2 |
Original Data | Converted Data Asplund et al. (2009) | |||||||
---|---|---|---|---|---|---|---|---|
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na I | 4 | ... | 0.22 | ... | -1.16 | 0.30 | 5.08 | Na I |
Mg I | 4 | ... | 0.39 | ... | -1.10 | 0.36 | 6.50 | Mg I |
Al I | 1 | ... | -0.55 | ... | -2.00 | -0.54 | 4.45 | Al I |
Fe | N/A | -1.47 | ... | ... | -1.46 | ... | 6.04 | Fe |
Right Ascension : 08 44 24.69 | Declination : +24 47 47.7 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
N/A | FOCES | 40000 | 200 | 2400 | N/A |